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NEAR-IR PHOTOMETRIC AND OPTICAL SPECTROSCOPIC STUDY OF THE FU ORIONIS OBJECT V582 AURIGAE

  • OH, HYUNG-IL (Department of Astronomy and Atmospheric Sciences, Kyungpook National University) ;
  • YOONY, TAE SEOG (Department of Astronomy and Atmospheric Sciences, Kyungpook National University) ;
  • SUNG, HYUN-IL (Korea Astronomy and Space Science Institute)
  • Received : 2014.11.30
  • Accepted : 2015.06.30
  • Published : 2015.09.30
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Abstract

We carried out near-IR photometric and optical spectroscopic observations of V582 Aur, which is a FU Orionis type object, to investigate any periodic and/or aperiodic variations. We obtained light curves on the scale of a night and a year, in J, H and Ks bands with KASINICS (KASI Near Infrared Camera System) attached to the BOAO (Bohyun-san Optical Astronomy Observatory) 1.8-m reflector in Youngcheon, South Korea and examined photometric variations on the two time scales. So far we have not found any periodic brightness variations on the scale of a night. On the other hand, we have found that there seems to be a periodic brightness variation with a period of approximately 45 days. In addition, high-resolution optical spectroscopic observations of V582 Aur were performed from February 2013 to May 2014 with the high-resolution echelle spectrograph BOES attached to the BOAO 1.8-m reflector. We analyzed several spectral lines to understand the physical state of V582 Aur. The P Cyg profiles are clearly shown in the $H{\alpha}$ line and Na I D line.

Keywords

Acknowledgement

Supported by : National Research Foundation of Korea (NRF)

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Cited by

  1. An UXor among FUors: Extinction-related Brightness Variations of the Young Eruptive Star V582 Aur vol.853, pp.1, 2018, https://doi.org/10.3847/1538-4357/aaa242